[meteorite-list] About the meteorite of Prambachkirchen, in GERMAN!

2006-10-21 Thread Peter Marmet


http://www.nachrichten.at/magazin/erforscht/486940? 
PHPSESSID=2bb12ad4e467bfc383fc435f07f7ef4e


Peter


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[meteorite-list] Is that beer on your tie? (yes, on-topic)

2006-10-21 Thread Darren Garrison
Don't know if they are serious about the mention of meteorites or not, but if so
some of us might want to take them up on the offer.

http://www.the-scientist.com/news/display/25122/;jsessionid=448543B377A09AAA4E7FF120AC9CB3BF

Is that beer on your tie?
A molecular biophysicist helps fund his lab with lush microphotos that decorate
neckties, calendars and greeting cards

[Published 20th October 2006 03:41 PM GMT]

In Michael Davidson's photographs, a Tylenol pill looks like a tie-dyed
explosion, a drop of Pina Colada appears to be an array of peacock feathers, and
an Intel microprocessor resembles a futuristic urban map. To achieve these
effects, he gets close to his subjects -- really close. 

For the past 35 years, the molecular biophysicist, who heads up the Microscopy
Office at Florida State University's National High Magnetic Field Laboratory,
has captured the intricate universes under his microscope slides and developed
them into vivid works of abstract art. The lush images have been reproduced on
neckties, calendars, sportswear, and greeting cards. 

Though he never studied art or photography, Davidson has landed an astonishing
1,500 magazine covers. And his lab's artistic arm, Molecular Expressions, has
created nearly 750,000 images, including microphotos of DNA, vitamins,
pharmaceuticals and beer, to name a few. (The lab is always looking for original
samples. Should you have any dinosaur bones or meteorites lying around and be
willing to make a short-term loan, they'll deliver free color microprints of the
objects in return.) 

The team is well versed in technologies ranging from confocal microscopy to
live-cell imaging, but turning science into art presents a new set of technical
challenges. To create his striking images, Davidson had to find ways to bridge
the gap between what he saw through his microscope and what the camera lens saw.
Because the eye detects more fluctuations along the color spectrum, the
challenge has been creating specimens that work as well for the camera as they
do for the human eye. For starters, the molecules have to be in crystalline
form, so that they will generate the contour-revealing colors of polarized
light. 

In a touch of poetic justice, it's the defects that reveal the most striking
designs and patterns. A flawless diamond would just look like a mirror under
the microscope, Davidson said. 

Preparing the specimens can take weeks or months. Davidson's expansive
collection of microimages of beer, for example, was particularly grueling to put
together. A lot of beers are pretty close to one another, chemically speaking,
he explained. Only a few motifs are different, yet we had to assign a distinct
pattern to each brand. 

Once the specimen is ready, an understanding of composition is essential to good
microphotography, said Davidson, who now uses digital instruments to snap the
shots. The way a photograph is framed has a dramatic impact, he said, noting
that that's what he most impresses upon his lab employees, now that he has
stepped into a less hands-on role in the microphotography enterprise. Rather
than do it myself, I critique the others. I'm trying to generate baby Picasso
microphotographers! 

When not honing their aesthetic sense, the lab members are developing
microscopic techniques. In September, Davidson and colleagues published a report
in Science on photo-activation location microscopy, which enables researchers to
see high-resolution single molecules in biological structures. 

Despite the success of his microphotography venture, Davidson said he still sees
the art as primarily a way to fund his science habit. It was a matter of
survival at first; we had been working for funding from NIH for so long. And
then we found we could sell these photos and make more money than I ever
imagined. The neckties alone brought in $1.5 million in the 1990s, with the
beer and cocktail images being the hottest sellers. 

Much of the profits were reinvested in lab equipment and used to launch its
extensive educational websites for students of all levels of microscopy.
Davidson's broader mission is to use his compelling images to generate interest
in science. Someone's not likely to read a paragraph on vitamin D, but if they
see a beautiful picture of it next to the [paragraph], they are more likely to
read it. 

Still, some of the most beautiful things in science, you can't slap up as a
photograph, Davidson said. Take line DNA replication. It's so complex. The
multiple mechanisms are just incredible. Far more beautiful than any photo I
have taken. 
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RE: [meteorite-list] Re: Ad New Lunar Seymchan Bessey Specks

2006-10-21 Thread E.P. Grondine
Hi Mike, list - 

Just when Bessey Specks were finally out of my
conciousness, along comes another cut lunar - 

Okay. How about cuttings as in cuttings from NWA999
Lunar/Martian meteorite preparation by  as an
alternative to Bessey Specks? Put that on the tag
alongside your picture of the Moon or Mars, and that
way both the rock and the preparer get credit, if the
child ever reads it carefully as he grows up.

lunar cuttings 
martian cuttings

cuttings  Now sell at Air  Space, Houston, Kennedy
in those child proof little acrylic bullion holders
Anne showed.

arghh - enough: a neologism and perhaps a new market.
Maybe the IMCA could organize this

good hunting,
Ed
Man and Impact in the Americas







--- MARK BOSTICK [EMAIL PROTECTED] wrote:

 
 That 146.4 gram Seymchan piece is just awesome Mike.
 
 http://jensenmeteorites.com/Seymchan.htm
 
 
 Clear Skies,
 Mark Bostick
 www.meteoritearticles.com
 
 
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[meteorite-list] Tuscon show dates

2006-10-21 Thread steve arnold
test

Steve Arnold,Chicago,USA!!
BIG Steve's Meteorites,1999!!

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[meteorite-list] (no subject)

2006-10-21 Thread steve arnold
test

Steve Arnold,Chicago,USA!!
BIG Steve's Meteorites,1999!!

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[meteorite-list] new email address

2006-10-21 Thread steve arnold
Hi list.I have a new email address.It is
[EMAIL PROTECTED] update your
records.Thanks and have a great day.






steve arnold,chicago


Steve Arnold,Chicago,USA!!
BIG Steve's Meteorites,1999!!

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[meteorite-list] email to the list from Phil Mani

2006-10-21 Thread Paul Harris

Dear List,
Phil was having difficulties getting his email to post to the list so 
I am forwarding it for him.


From: mailto:[EMAIL PROTECTED]Philip mani
To: 
mailto:Meteorite-list@meteoritecentral.comMeteorite-list@meteoritecentral.com 


Sent: Saturday, October 21, 2006 9:13 AM
Subject: Brenham Project

This letter is my first post to the Meteorite List after being a 
long-time reader.  I am the fortunate beneficiary of much recognition 
from so many of you related to my Brenham Project with Steve 
Arnold.  Thank you for your kind words and encouragements.  With this 
posting, I wanted to publicly recognize certain individuals who are 
the main contributors, in my opinion, to our most recent expedition 
and without whose efforts and creativity the wonderful story written 
by Associated Press would not have been possible.


It was last July when I began conversations with Carolyn Sumners, 
Director of Astronomy of the Houston Museum of Natural Science.  I 
offered HMNS an opportunity to join Steve and I in Kansas on a 
meteorite search and recovery project.  Mrs. Sumners was excited 
about the opportunity and asked me what specifically HMNS could 
contribute as far as unanswered questions about the find.  I told her 
we questioned the timing/age-date assigned to the fall and we wished 
to try to pin-down its timing.  We discussed several methods for 
age-dating and left her and her experts to further discuss and 
implement the methods for age-dating.  A second question is the 
direction of the meteorite fall, specifically, its bearing and 
descent angle.  This question is more complex and we felt we needed 
to gather as much survey information as possible without disturbing 
the meteorites and the soil around them.  At this point, Mrs. Sumners 
contacted Dr. Essam Heggy with the Lunar Planetary Institute 
regarding his ground penetrating radar work.


I informed Steve and he said he would do his best for the museum.  I 
remained convinced he could find another meteorite.


After all details with the HMNS, LPI, and our landowners were worked 
out, I contacted our good friend, Darryl Pitt, to assist with all 
facets for release of information to the public regarding this expedition.


You all know our results.

Steve was able to pull the golden rabbit out of the hat.  My sincere 
appreciation and congratulations to him once again and, if you have 
seen the strewnfield you understand why.  He tells me he feels his 
ability to do so again from this point on will be less and 
less.  Therefore, our search and recovery efforts for Brenham 
meteorites is beginning to wind-up.


Carolyn Sumners' group from HMNS included astronomers, geologists, 
paleontologists and archeologists with long and storied excavation 
and recovery experiences.  It was a joy and a treat to be an observer 
of their efforts.  I am excited for them and their unique meteorite 
recovery.  Good going.


Dr. Heggy, with LPI, was faced with a substantial change of 
conditions from those he originally anticipated in the 
field.  Southwest Kansas had received quite a bit of rain and in the 
last three days, we were in constant heavy drizzle, blown sideways by 
20-plus mile an hour winds.  If not for the excitement of the project 
and all involved, it would have been miserable to be in such 
conditions for the 12 or more hours per day.  Dr.  Heggy adapted his 
equipment and techniques and continued to proceed as diligently as 
the rest of us without becoming discouraged.  His efforts too were rewarded.


Finally, but certainly not least, Darryl Pitt single-handedly 
prepared the initial press release and then he, along with the 
brilliant efforts of a colleague of his in New York, facilitated the 
amazing Associated Press story by Roxana Hegeman.  Darryl worked 
closely with Roxana a day or two before Monday's final excavation of 
the museum's 154-pound pallasite and she was very well prepared for 
what to expect on the final day.  It was only yesterday evening I 
learned that Roxana's story has enjoyed the widest world-wide 
distribution of any story ever pertaining to meteorites (with the 
exception of the announcement of ALH84001).  Certainly amazing.


I am grateful to be a part of the Brenham Project.  I have learned 
much more than I ever anticipated being a meteorite collector.  This 
particular chapter of our project was such a treat to watch 
unfold.  I am reminded of Greg's words to the List that this is an 
awesome story where meteorite hunters, collectors and scientists can 
join to work together closely in the field using new equipment to 
make a wonderful meteorite recovery.  I am blessed to have participated.


Congratulations to Carolyn Sumners and her HMNS team for their 
thoughtful work and the additional, continuing work to come both in 
age-dating the fall and hopefully determining the fall direction and angle.


Great-going Dr. Heggy for your successful use and application of the GPR.

Hats-off to Darryl for facilitating the 

[meteorite-list] Chondrule formation mechanism

2006-10-21 Thread E.P. Grondine
Hi all - 

I think I would be right in saying that the usual
mechanism proposed for chondrule formation is
precipitation at low temperatures over time.

But I am wondering: could chondrule formation be
linked to the release of pressure?  Could it be like a
soda-pop, where when you take the cap off the CO2
becomes bubbles?  Could chondules be mineral bubbles
which formed when pressure was released on an
immiscible suspension?

It is often stated that there are no stupid questions,
and I hope I have not provided an example to the
contrary with this one.

good hunting,
Ed





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Re: [meteorite-list] Chondrule formation mechanism

2006-10-21 Thread Darren Garrison
On Sat, 21 Oct 2006 10:12:56 -0700 (PDT), you wrote:

I think I would be right in saying that the usual
mechanism proposed for chondrule formation is
precipitation at low temperatures over time.

No, actually it isn't.  Chondrules are usually proposed to be products of rapid
melting. 
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Re: [meteorite-list] Portales Valley Q

2006-10-21 Thread Michael L Blood
Does anyone on the list know the current status
of classification for Portales Valley? When it first
fell, I believe it was merely classified as (H6), which
I thought was insulting to one's logic. Then, I heard
the classification had been changed (about time). However,
I recently saw a Michael Cottingham card that read,
(H7)? That seemed to me to be, indeed, odd.
So, does anyone KNOW?
Also, is there a DIFFERENT classification for the
low metal vs high metal forms - or did the new
classification address that?
I am sure many list members would be interested
to know.
Thanks, Michael









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Re: [meteorite-list] Portales Valley Q

2006-10-21 Thread Robert Woolard
Hello Michael and List,

  I don't have a final, definitive answer to your
question. It is one that I, too, have been seeking an
answer to for a long time. 

   Here is a link to a fairly recent article that
raises some good points:

 
http://www.psrd.hawaii.edu/Sept05/PortalesValley.html


  Robert Woolard

   






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Re: [meteorite-list] Portales Valley Q

2006-10-21 Thread David Weir

Michael,

This was the subject on the list just a year ago. I had expressed my 
favor of the journal article by A. Ruzicka et al. (2005), which referred 
to PV by a new term -- H-chondrite, metallic-melt breccia. Jeff Grossman 
posted the following in reply, which actually does seem like a 
completely logical classification based on the petrogenesis proposed in 
the above paper:


--
Obviously there is disagreement among scientists
on what to call PV.  I personally see no reason
to call it type 7, a primitive achondrite, an
achondrite OR to coin a new term.  If I take the
conclusions of the Ruzicka study as a given, that
you had H6 material near its peak metamorphic
temperature, which additional shock heating and
mobilization of metal-rich melt, then I see no
reason not call it an H chondrite impact melt
breccia in which the clasts are dominantly type 6.

jeff
-

David
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[meteorite-list] nearly nailed part three

2006-10-21 Thread Bob WALKER

Hi listees

A fellow member was asking me if I recalled the name of a meteorite fall 
where a guy got mud splattered on him...


My few remaining pieces of grey matter remind me that ENSISHEIM fits into 
this category but are list members aware of any other falls with similar 
circumstances - please post names of same to the list or message me


Cheers 


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[meteorite-list] AD: EBAY NWA CLEARING OUT SALE

2006-10-21 Thread dean bessey
I have been pretty quite meteorite wise lately and
didnt feel like updating my website for sold items so
I have listed a couple hundred meteorites on ebay.
These are mostly items that I have offered in the past
but in an effort to clear out old stock, get ready for
new meteorites next month, and to raise money for
munich I have significantly reduced prices on
everything - large proportions of my current ebay
listings are under 10 cents a gram.
See my ebay id AMUNRE or click here:
http://stores.ebay.com/AMUNRE-COLLECTIBLES-AND-GEMSTONES_Meteorites_W0QQcolZ4QQdirZ1QQfsubZ4QQftidZ2QQtZkm
Or if its to long this should work also:
http://tinyurl.com/y5myap
Sincerely
DEAN BESSEY
http://www.meteoriteshop.com

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[meteorite-list] BESSEY SPECK INFORMATION NOW ON EBAY

2006-10-21 Thread dean bessey
In light of the recent discussion on this list about
Bessey Specks and in the interest of new list members
who were not around a few years ago when bessey specks
came into existance I have listed this ebay auction to
explain how it all started (And your chance to get
your very own Bessey Speck).
See my ebay auction #190043654452
Or click here:
http://cgi.ebay.com/ws/eBayISAPI.dll?ViewItemcategory=3239item=190043654452
Sincerely
DEAN BESSEY
http://www.meteoriteshop.com


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[meteorite-list] Polandmet auctions ending OT AD

2006-10-21 Thread PolandMET

Hi again.
15 auctions ending in 24 hours including
CV3
CV3-anomalous
CR2
ODIO
L6 IMB
L3.1

http://cgi.ebay.com/ws/eBayISAPI.dll?ViewItemrd=1item=110044409830
This piece make me realy crazy. I have cut some ordinary meteorite 
fragments. I could expect anything special in this low quality material 
except rust, missing iron and dark matrix.

But then a big surprize. One of my most lucky cuts I have ever made.
I have cut this specimen just perfect into center of a large chondrule.
Im not 100% sure , but this one looks like extra large 10x8 mm chondrule.

Let me know what is Your opinion about this object.

Visit my eBay shop
http://stores.ebay.com/PolandMET-Store

-[ MARCIN CIMALA ]-[ I.M.C.A.#3667 ]-
http://www.Meteoryt.net [EMAIL PROTECTED]
http://www.PolandMET.com   [EMAIL PROTECTED]
http://www.Gao-Guenie.com  GSM +48(607)535 195
[ Member of Polish Meteoritical Society ]

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Re: [meteorite-list] Chondrule formation mechanism

2006-10-21 Thread E.P. Grondine
Hi Darren  - 

Thanks - much has been lost in the stroke. I also seem
to remember a long slow cooling involved in 
chondrule formation - 

I am thinking that effervescence following a sudden
release of pressure might be a better process
description - 

good hunting,
Ed

--- Darren Garrison [EMAIL PROTECTED] wrote:

 On Sat, 21 Oct 2006 10:12:56 -0700 (PDT), you wrote:
 
 I think I would be right in saying that the usual
 mechanism proposed for chondrule formation is
 precipitation at low temperatures over time.
 
 No, actually it isn't.  Chondrules are usually
 proposed to be products of rapid
 melting. 
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Re: Re: [meteorite-list] Chondrule formation mechanism

2006-10-21 Thread Darren Garrison
On Sat, 21 Oct 2006 14:58:23 -0700 (PDT), you wrote:

Hi Darren  - 

Thanks - much has been lost in the stroke. I also seem
to remember a long slow cooling involved in 
chondrule formation - 


Googling chondrule formation comes up with lots of stuff, much of it pretty
densly technical.  Here's one interesting tidbit (unfortunately you have to buy
the whole article to read it):

 http://www.aspbooks.org/custom/publications/paper/index.phtml?paper_id=2447

Chondrule textures depend on the extent of melting of the chondrule precursor
material when cooling starts. If viable nuclei remain in the melt,
crystallization begins immediately, producing crystals with shapes that approach
equilibrium. If not, crystallization does not occur until the melt is
supersaturated, resulting in more rapid growth rates and the formation of
skeletal or dendritic crystals. A chondrule texture thus indicates whether
nuclei were destroyed, which implies a melting temperature above the liquidus
temperature for its particular composition. The presence or absence of skeletal
or dendritic crystals in chondrules can be used to constrain their peak
temperatures, which range from 1400-1850°C. Heating times of less than a second
result in aggregates of starting materials coated with glass, resembling
agglutinates rather than objects with typical chondrule textures, suggesting
that heating times are longer. Chondrule textures can be duplicated with a very
wide range of cooling rates, but if olivine zoning is to be matched the cooling
rate should be within the range 10- 1000°C/hr. The size of overgrowths on relict
grains cannot be used to infer cooling rates. Chondrules melted in a canonical
nebular gas lose sulfur and alkalis in minutes, while iron loss from the
silicate melt continues over many hours. Mass loss and isotopic fractionation
can be suppressed if the partial pressures of the species of interest are high
enough in the ambient gas. Chondrule bulk and mineral composition arrays can be
reproduced to a large extent by evaporation. However, condensation of SiO into
the melt can simulate the zonation in some chondrules, with pyroxene and a
silica polymorph near the rims. The partial equilibration of chondrule melt with
noncanonical nebular gas would require heating for time periods of hours. 


I am thinking that effervescence following a sudden
release of pressure might be a better process
description - 

Hm.  Effervescence following a sudden release of pressure makes me think more of
a can of Coke.  :-)
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Re: [meteorite-list] Permian-Triassic Mass Extinction Cause: 'SickEarth'

2006-10-21 Thread Sterling K. Webb

Hi, All,

   Ah, press-release-science! The part of such
announcements that is annoying is that there is
no room in a press release for evidence, unless
it's one piece of new-discovery evidence. None
of that here. It's a theory...

   So, as I read the (by now) many press pieces
on Sick Earth Syndrome. I assume that there
must a good record of long-term variations and
declines in Permian oxygen levels. That's certainly
what the articles imply.

   I went a-Googling to find such a record, and --
guess what? -- there isn't one. The Permian was
an oxygen rich period mostly. There IS a record of
an event covering less than a half million years
which shows a thin layer with a sudden and dramatic
drop in oxygen accompanied by a dramatic marine
extinction, then a thicker layer showing a partial
recovery to still-low oxygen levels accompanied
by continuing extinction at a lesser rate, followed
a layer that begins the oxygen boom of the Triassic.
http://palaeo.gly.bris.ac.uk/Essays/wipeout/default.html

   This, of course, is EXACTLY what I (for example)
would expect the record of the biggest impact of the
last half-billion years to look like. I don't think that
a half-million years is very long to recover from such
an immense whack! But the palaeontologists are saying
(in effect) that it can only be an asteroid disaster if
the dramatic aftermath of a major impact are limited
to the eye-blink of a fruit bat in time. In geologic terms,
they're demanding we find a discontinuity but no
after effects.

   All these changes -- sulfate events, methane events,
dramatic climate change up, down and sideways, with
erratic atmospheric gas levels -- are perfectly explained
by an impact's effect on the Earth, particularly since
they're crammed into a short time span. The geologists
have a short time span event to blame: the flood basalts
of the Siberian Traps. Now, if they had the vaguest idea
what causes giant basalt floods, they'd be in a better
position to thumb their nose at an asteroid... But they
don't know.

   We have flood basalt events all over the Solar
System, of course, and it's pretty obvious what
caused them. And we have a mechanism for flood
basalts on Earth having been caused by impacts
(focused shock waves). And the uncommonness
of flood basalts is on the same order as the
uncommonness of a Big Whack. Then, there are
the coincidences like Chicxulub and the Deccan
Traps, and this one, too.

   In the Permian, there was only one continent,
good old Pangea, and lots of shallow ocean everywhere
else. Since the Permian event was a largely marine
extinction (94% of all marine species) and the odds on
an asteroid striking ocean are good, that too is suspicious.
Ocean crust is nowhere older than 200 million years,
so direct evidence (crater) of an ocean strike is gone.
Marenco's long-term sulfur isotope variations are
fully explicable in terms of the changes in continents
and oceans but are they great enough to wipeout
nearly all life?

   For 5 million years after the Event, there is no
evidence of the existence of coral reefs. Note that
this not the absence of the coral animals that build
them, but the absence of the reefs themselves. OK,
I can believe that sulfite killed the coral critters, but
explain to me how it removed all their housing as
well? I have trouble with that. Of course, the biggest
tidal wave in a billion years could sweep away their
reefs, no problem... Corals came back, obviously,
but it took them 20-30 million years. Sounds like
they had to bulding all-new housing from scratch,
doesn't it? AND, the continental configuration that
supposedly caused all this difficulty hadn't changed
one bit in the intervening time! If the continental
configuration can cause a mass extinction, why
didn't it keep on causing it? Change of heart?

   The half-million years of trouble marked by China's
Bed 25, 26, and 27 is only 30 cm thick and the layer
that shows the disaster (#25) is only 5 of those 30
centimeters, or about 80,000 years worth at uniform
rates of depositation. Of course, Bed 25 could be
from 10,000 years of depositation, too, or even only
1000 years.

   All these timescales are too short to date at
251 million years in the past. Layer 25 is full of
evidence of the Siberian Traps vulcanism, and that
surely went on a while. So, the sharpness of
the triggering event is not determinable. And the
iridium layer, if there even was one, would be
lost in it, as would most extraterrestrial markers
('cept the gasses in the buckeyballs?).

   I don't know if the Wilkes Land Crater will pan
out, nor Becker's Buckyballs, but if this were Las
Vegas, I would still put my money on the Permian
Whacker (knockout in the first round) over the
Siberian Gassy Wipeout as The Winnah!


Sterling K. Webb
--
- Original Message - 
From: Ron Baalke [EMAIL PROTECTED]

To: Meteorite Mailing List meteorite-list@meteoritecentral.com
Sent: Friday, October 20, 2006 3:52 

Re: Re: [meteorite-list] Chondrule formation mechanism

2006-10-21 Thread E.P. Grondine
Thanks Darren - 

now this is more like it - h

--- Darren Garrison [EMAIL PROTECTED] wrote:

http://www.aspbooks.org/custom/publications/paper/index.phtml?paper_id=2447
 
 Chondrule textures depend on the extent of melting
 of the chondrule precursor- material when cooling 
 starts. 

Kind of begs the question - chodrules formed by
collision, which causes melt - consider if one started
from a steady molten state 

If viable nuclei 

I wonder what these viable nuclei are? viable cystal
nuclei=Chondrules?

 remain in the melt, crystallization begins 
 immediately, producing crystals with shapes that 
 approach equilibrium. If not, crystallization does
 not occur until the melt is supersaturated,
resulting
 in more rapid growth rates and the formation of 
 skeletal or dendritic crystals. 

 A chondrule texture thus indicates whether
 nuclei were destroyed, which implies a melting
 temperature above the liquidus temperature for its
 particular composition. The  presence or absence of 
 skeletal or dendritic crystals in chondrules can be 
 used to constrain their peak temperatures, which 
 range from 1400-1850°C. 

hmmm - collision temperatures of 1400-1850°C

 Heating times of less than a second result in 
 aggregates of starting materials coated
 with glass, resembling agglutinates rather than
 objects with typical chondrule textures, suggesting
 that heating times are longer. 

different heating times=two mechanisms for chondrule
formation?  two classes 1)agglutinate 2)original?

 Chondrule textures can be duplicated with a very
 wide range of cooling rates, but if olivine zoning
 is to be matched the cooling rate should be within
 the range 10- 1000°C/hr. The size of overgrowths on 
 relict grains cannot be used to infer cooling rates.


 Chondrules melted in a canonical nebular gas lose 
 sulfur and alkalis in minutes, while iron loss from
 the silicate melt continues over many hours. Mass
 loss and isotopic fractionation can be suppressed if
 the partial pressures of the species of interest are
 high enough in the ambient gas. Chondrule bulk and
 mineral composition arrays can be reproduced to a 
 large extent by evaporation.

Yeah, but chondrules are found in matrices.

 However, condensation of SiO 

and how exactly is this SiO condensation supposed to
occur?

 into the melt can simulate the zonation in some
 chondrules, with pyroxene and a silica polymorph
near  the rims. 

yeah, but could the silica rims have come from the
inside?

 The partial equilibration of chondrule melt with
 noncanonical nebular gas would require heating for
 time periods of hours. 

 Hm.  Effervescence following a sudden release of
 pressure makes me think more of
 a can of Coke.  :-)

We all get our inspiration somewhere - 

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[meteorite-list] Radar locates meteortite story in LA Times.

2006-10-21 Thread doctor death

Where do I get my radar gun?

http://www.latimes.com/technology/la-sci-meteorite21oct21,0,307156.story?coll=la-home-headlines

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Re: [meteorite-list] Chondrule formation mechanism

2006-10-21 Thread Darren Garrison
On Sat, 21 Oct 2006 16:41:48 -0700 (PDT), you wrote:

 Chondrule textures depend on the extent of melting
 of the chondrule precursor- material when cooling 
 starts. 

Kind of begs the question - chodrules formed by
collision, which causes melt - consider if one started
from a steady molten state 

If viable nuclei 

I wonder what these viable nuclei are? viable cystal
nuclei=Chondrules?

How things appear to be (without trying to refer to chemical/minerological
details that are beyond my level of knowledge) is that what became chondrules
started out as fluff that slowly accumulated from the solar nebula, like you
mentioned earlier.  I imagine something like snowflakes, or dust-bunnies.
Something fragile and irregular filled with empty spaces.  Then, something (and
there is no consensus on what that something was) heated those
dust-bunnies/snowflakes up to the point where they melted-- and in a
microgravity environment surface tension pulled them into little spheres.  The
viable nuclei means parts of that original fluff that didn't fully melt and
became seeds for the new minerals to grow on.
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Re: [meteorite-list] Radar locates meteortite story in LA Times.

2006-10-21 Thread Darren Garrison
On Sat, 21 Oct 2006 17:56:51 -0600, you wrote:

Where do I get my radar gun?

Can the radar be tuned to find other types of stories in other publications?
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Re: [meteorite-list] Chondrule formation mechanism (Info Please)

2006-10-21 Thread Rob McCafferty
Hi list

What I have ben able to find personally on chondrule
formation is rather sketchy. 

Even the otherwise comprehensive Encyclopedia of
Meteorites by O. Richard Norton seems to skim over the
mechanism in a paragraph. It's almost as if there is
something which defies explanation and scientists
abhor that more than nature abhors a vacuum.

The slow cooling followed by a rapid quenching
period is that which interests me most. 

I would dearly like to know where to find the most
up-to-date theories on chondrul formation. I know
about the R-R Lyrae heating, timescales and frequecies
for newly forming stars. I need theory of protostellar
nebula. Maybe Nebula density/stellar distance formula.
The conditions in which and the timescale in which
these 0.1- 3mm chondules formed. 

Contact off list if you wish. I need this information
to assist me with a theory I have, the information for
which comes from branches of science so diverse, that
their relevance has not been realised. It is only by
serendipity that I make the connection.
My thoughts will appear here first (though I will
ruthlessly hunt down and murder anyone who tries to
plagarise my theory, hehe)

Rob McCafferty

 
--- Darren Garrison [EMAIL PROTECTED] wrote:

 On Sat, 21 Oct 2006 16:41:48 -0700 (PDT), you wrote:
 
  Chondrule textures depend on the extent of
 melting
  of the chondrule precursor- material when cooling
 
  starts. 
 
 Kind of begs the question - chodrules formed by
 collision, which causes melt - consider if one
 started
 from a steady molten state 
 
 If viable nuclei 
 
 I wonder what these viable nuclei are? viable
 cystal
 nuclei=Chondrules?
 
 How things appear to be (without trying to refer to
 chemical/minerological
 details that are beyond my level of knowledge) is
 that what became chondrules
 started out as fluff that slowly accumulated from
 the solar nebula, like you
 mentioned earlier.  I imagine something like
 snowflakes, or dust-bunnies.
 Something fragile and irregular filled with empty
 spaces.  Then, something (and
 there is no consensus on what that something was)
 heated those
 dust-bunnies/snowflakes up to the point where they
 melted-- and in a
 microgravity environment surface tension pulled them
 into little spheres.  The
 viable nuclei means parts of that original fluff
 that didn't fully melt and
 became seeds for the new minerals to grow on.
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[meteorite-list] Henbury Auction Ending Today - AD

2006-10-21 Thread Jeff Kuyken
G'day,

Just a reminder that there's a nice 220g Henbury individual ending today.
Nice specimens around this size are extremely difficult to get in Australia
now and this one is currently going for a fraction of its value!

http://cgi.ebay.com/ws/eBayISAPI.dll?ViewItemih=002item=120042289479

Cheers,

Jeff

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[meteorite-list] Rocks From Space Picture of the Day - October 22, 2006

2006-10-21 Thread SPACEROCKSINC
http://www.spacerocksinc.com/October_22.html  

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Re: [meteorite-list] Chondrule formation mechanism (Info Please)

2006-10-21 Thread E.P. Grondine
jeez Bob, 

and all I was trying to do was to come up with a good
excuse to personally examine that Krasnojarsk RSPOD
Oct 15.  

You're just about ready to handle some of my asteroid
and comet impact correspondence.

Ed

--- Rob McCafferty [EMAIL PROTECTED] wrote:

 Hi list
 
 What I have ben able to find personally on chondrule
 formation is rather sketchy. 
 
 Even the otherwise comprehensive Encyclopedia of
 Meteorites by O. Richard Norton seems to skim over
 the
 mechanism in a paragraph. It's almost as if there is
 something which defies explanation and scientists
 abhor that more than nature abhors a vacuum.
 
 The slow cooling followed by a rapid quenching
 period is that which interests me most. 
 
 I would dearly like to know where to find the most
 up-to-date theories on chondrul formation. I know
 about the R-R Lyrae heating, timescales and
 frequecies
 for newly forming stars. I need theory of
 protostellar
 nebula. Maybe Nebula density/stellar distance
 formula.
 The conditions in which and the timescale in which
 these 0.1- 3mm chondules formed. 
 
 Contact off list if you wish. I need this
 information
 to assist me with a theory I have, the information
 for
 which comes from branches of science so diverse,
 that
 their relevance has not been realised. It is only by
 serendipity that I make the connection.
 My thoughts will appear here first (though I will
 ruthlessly hunt down and murder anyone who tries to
 plagarise my theory, hehe)
 
 Rob McCafferty
 
  
 --- Darren Garrison [EMAIL PROTECTED] wrote:
 
  On Sat, 21 Oct 2006 16:41:48 -0700 (PDT), you
 wrote:
  
   Chondrule textures depend on the extent of
  melting
   of the chondrule precursor- material when
 cooling
  
   starts. 
  
  Kind of begs the question - chodrules formed by
  collision, which causes melt - consider if one
  started
  from a steady molten state 
  
  If viable nuclei 
  
  I wonder what these viable nuclei are? viable
  cystal
  nuclei=Chondrules?
  
  How things appear to be (without trying to refer
 to
  chemical/minerological
  details that are beyond my level of knowledge) is
  that what became chondrules
  started out as fluff that slowly accumulated
 from
  the solar nebula, like you
  mentioned earlier.  I imagine something like
  snowflakes, or dust-bunnies.
  Something fragile and irregular filled with empty
  spaces.  Then, something (and
  there is no consensus on what that something
 was)
  heated those
  dust-bunnies/snowflakes up to the point where they
  melted-- and in a
  microgravity environment surface tension pulled
 them
  into little spheres.  The
  viable nuclei means parts of that original fluff
  that didn't fully melt and
  became seeds for the new minerals to grow on.
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[meteorite-list] Need Source For Bulk Tektites

2006-10-21 Thread Ed Deckert

Hi everyone,

I am trying to obtain a source for bulk quantities of Tektites.  Not too 
small, but not huge either.  Perhaps the size of a US 25 cent piece at the 
very smallest, and at the most, up to the size of 3 US 25 cent pieces in a 
triangular configuration, or 4 of them side by side in a 2 x 2 matrix.  I 
need them to be in good condition (not all bashed or chipped up from being 
tossed about in collecting buckets, or from being shipped all over the 
place.)  And the price has to be really good (super cheap) too.  Yeah - I 
know it sounds like I've been smoking funny cigarettes, but let me assure 
you, I have not.  Well, at least I can't remember doing that...;-)


Why do I need them?  I am coordinating a fund raiser for my local astronomy 
club.  I already have some nice unclassified NWA Meteorites, plus some nice, 
relatively inexpensive NWA 4293 that I am going to donate to the cause.  So, 
OK - I have the Meteorites covered - but I want to add some Tektites to this 
as well.  We figure that we can sell these at club events, and they can also 
be donated to school teachers without breaking the bank.  We want to share 
education with respect to astronomy, meteorites, and basically any aspect of 
the hobby, and hopefully foster the growth of interest in astronomy in the 
community (kids, especially) and recruit some members.


How much am I looking for?  I would like to obtain a couple of kilos.  I 
suppose shipping them can result in a little bit of chipping in transit, so 
that may be an unavoidable problem.


If anyone can let me know where I can find a good, and inexpensive Tektite 
source, I would really appreciate hearing from you.


Best regards,

Ed Deckert


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[meteorite-list] A probable iron meteorite fall in Italy many time ago

2006-10-21 Thread M come Meteorite Meteorites
Hello

Today my goldsmith have show to me 2 little rounded 
balls  of iron with a grey dark crust well visible
and some rust. He have say its of a person have take
this 2 pieces many years ago after this is fall near
the house of this person. The rust have the tipycal
smell of the meteorites rust - its many different from
the terrestrial rust - unfortunately the person not
want cut one of the 2 pieces for seen if the cut face
show the patterns why he want build this in a jewerly,
but probably a nichel test its possible for seen if is
a probable meteorite.

Matteo

M come Meteorite - Matteo Chinellato
Via Triestina 126/A - 30173 - TESSERA, VENEZIA, ITALY
Email: [EMAIL PROTECTED]
Sale Site: http://www.mcomemeteorite.it 
Collection Site: http://www.mcomemeteorite.info
MSN Messanger: spacerocks at hotmail.com
EBAY.COM:http://members.ebay.com/aboutme/mcomemeteorite/

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[meteorite-list] Brenham Project

2006-10-21 Thread Philip mani




This letter is my first post to the Meteorite List 
after being a long-time reader. I 
am the fortunate beneficiary of much recognition from so many of you related to 
my Brenham Project with Steve Arnold. 
Thank you for your kind words and encouragements. With this posting, I wanted to publicly 
recognize certain individuals who are the main contributors, in my opinion, to 
our most recent expedition and without whose efforts and creativity the 
wonderful story written by Associated Press would not have been 
possible.

It was last July when I began conversations with 
Carolyn Sumners, Director of Astronomy of the Houston Museum of Natural 
Science. I offered HMNS an 
opportunity to join Steve and I in Kansas on a meteorite search and recovery 
project. Mrs. Sumners was excited 
about the opportunity and asked me what specifically HMNS could contribute as 
far as unanswered questions about the find. I told her we questioned the 
timing/age-date assigned to the fall and we wished to try to pin-down its 
timing. We discussed several 
methods for age-dating and left her and her experts to further discuss and 
implement the methods for age-dating. 
A second question is the direction of the meteorite fall, specifically, 
its bearing and descent angle. This 
question is more complex and we felt we needed to gather as much survey 
information as possible without disturbing the meteorites and the soil around 
them. At this point, Mrs. Sumners 
contacted Dr. Essam Heggy with the Lunar Planetary Institute regarding his 
ground penetrating radar work.

I informed Steve and he said he would do his best 
for the museum. I remained 
convinced he could find another meteorite.

After all details with the HMNS, LPI, and our 
landowners were worked out, I contacted our good friend, Darryl Pitt, to assist 
with all facets for release of information to the public regarding this 
expedition.

You all know our results. 

Steve was able to pull the golden rabbit out 
of the hat. My sincere appreciation 
and congratulations to him once again and, if you have seen the strewnfield you 
understand why. He tells me he 
feels his ability to do so again from this point on will be less and less. Therefore, our search and recovery 
efforts for Brenham meteorites is beginning to wind-up. 

Carolyn Sumners’ group from HMNS included 
astronomers, geologists, paleontologists and archeologists with long and storied 
excavation and recovery experiences. 
It was a joy and a treat to be an observer of their efforts. I am excited for them and their unique 
meteorite recovery. Good 
going. 
Dr. Heggy, with LPI, was faced with a substantial change of conditions 
from those he originally anticipated in the field. Southwest 
Kansas had received quite a bit of rain and in the last three days, 
we were in constant heavy drizzle, blown sideways by 20-plus mile an hour 
winds. If not for the excitement of 
the project and all involved, it would have been miserable to be in such 
conditions for the 12 or more hours per day. Dr. Heggy adapted his equipment and 
techniques and continued to proceed as diligently as the rest of us without 
becoming discouraged. His efforts 
too were rewarded.

Finally, but certainly not least, Darryl Pitt 
single-handedly prepared the initial press release and then he, along with the 
brilliant efforts of a colleague of his in New York, facilitated the amazing 
Associated Press story by Roxana Hegeman. 
Darryl worked closely with Roxana a day or two before Monday’s final 
excavation of the museum’s 154-pound pallasite and she was very well prepared 
for what to expect on the final day. 
It was only yesterday evening I learned that Roxana’s story has enjoyed 
the widest world-wide distribution of any story ever pertaining to meteorites 
(with the exception of the announcement of ALH84001). Certainly amazing.

I am grateful to be a part of the Brenham 
Project. I have learned much more 
than I ever anticipated being a meteorite collector. This particular chapter of our project 
was such a treat to watch unfold. I 
am reminded of Greg’s words to the List that this is an awesome story where 
meteorite hunters, collectors and scientists can join to work together closely 
in the field using new equipment to make a wonderful meteorite recovery. I am blessed to have 
participated.

Congratulations to Carolyn Sumners and her HMNS 
team for their thoughtful work and the additional, continuing work to come both 
in age-dating the fall and hopefully determining the fall direction and 
angle.

Great-going Dr. Heggy for your successful 
use and application of the GPR. 


Hats-off to Darryl for facilitating the AP wire 
story or, as I told him Tuesday morning when I learned it had already been 
picked up around the world “Wow! Wow! 
Wow! It’s 
amazing!”

To the List, so long for now. Steve and I are off to write another 
chapter for the Brenham Project and we intend to make it a good one. 

Very truly,

Phil Mani

Philip C. 

[meteorite-list] Ad World's smallest pocket scale

2006-10-21 Thread Mike Martinez





Hi Everyone

I have some wonderful scales for 
sale. I weighted a 241 gram 
meteorite on one and reweighed the same meteorite on an $1800.00 scale and it 
was accurate. That is incredible 
for something that can fit in your watch pocket. Check it out. 

http://www.meteorflash.com/SMALL.JPG


Pocket Scales  1/10th Gram 
 Key Chain Scale
$20.00 each, Shipping is free in the US 
and $3.00 overseas.

This is the world’s smallest pocket scale 
with slide cover. This compact 
scale is only 3” x 1.5” x 0.5”; and is small enough to be used as a key 
chain.

Although it’s tiny in size, it is fully 
functional with stainless steel platform and 
backlight.

It can be used in many applications 
i.e. Weighing food products for 
calorie control for a personal diet program, for weighing precious stones or 
gems for the weekend “rockhound” enthusiast or any other hobby where 1/10th gram 
accuracy is needed.

Product 
Features:

High quality strain gauge load cell system 
makes it accurate in full capacity range.

High density ABS housing and metal support 
makes it very durable.
Stainless steel platform is safer for food 
and more durable than competitor’s units with plastic 
platforms.
Detachable slide cover can be used as a 
scoop.
High contrasts LCD display makes the 
readouts clear to read.
TARE function covers unit’s full capacity 
range.
Attractive blue backlights make display 
easily readable in low light conditions.

Specifications:

Scale 
Size: 
3" (D) x 1.5" (W) x 0.5" (H) Weighing Modes: g/oz/ct/gn 
Capacity: 
DW-250BK: 250g 
Accuracy: 
0.1 gramPlatform 
Size:1.8" x 
1.2"Platform Material: Stainless steel LCD 
Size: 
1" x 0.3" 
Power:Two 
LR1130 lithium batteries 
(included)Packaging: 
100 per caseColors Available:Black, Silver, 
White

Regards

Mike Martinez

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Re: [meteorite-list] P-T Extinction: 'SickEarth' Book Recommendation

2006-10-21 Thread Mr EMan

What a segway! Based on what I read there was evidence
of a sick earth but Peter Ward's research showed a
very rapid extinction of land animals.

I just finished reading Gorgon: The Monsters That
Ruled the Planet Before Dinosaurs and How They Died in
the Greatest Catastrophe in Earth's History by Peter
Ward. Ward spent decades studing the Permian
Extinction in the Karoo district of South Africa. 
Ward was a specialist in the K-T extinction and looked
kept an eye out for a similar impact component. The
book is an account of the trials and tribulations of a
geologist trying to do science, make a living, and
raise a new family in the wilderness. The snobbbey and
blood-letting amongst researchers is insightful to the
way other researchers posion the pond in other fields.
The science is pretty neat. The book is rarely
predictible.  

Far too many dimentions to describe but the book is
cheap online and a must read for anyone interested in
the life of a geologist and novel solutions to solve
obsticles.

Ward's observations were that the land amimals that
survived and flourished ultimately were the ones which
had a bone structure that allowed for a flexible and
greater lung capacity--side slung arms aka
lizard-like.  Research supported that there was a
plunge in oxygen levels such that it was like moving
from sea level to 12000ft.  Part of the overall
observation is that Gondwana moved over the south pole
and in the ensuing ice age, sea level moved beyond the
already meger contentinal shelves cutting shallow
water habitat to nill killing the plankton bloom. The
sea based food chain collapsed along with the oxygen
production. There was a scarcity of land plants in the
Permian besause so much of the land mass was at the
interior of a massive water deprived landlocked
soiless landscape. Life in the Triassic remained meger
until the Breakup of Pangea opened up more shore line
to the interior.

The Siberian trapps at that time were above the
Artic(North) not far from where they are today.
 For a book description:
http://www.amazon.com/Gorgon-Paleontology-Obsession-Greatest-Catastrophe/dp/0670030945?tag2=gp04-20
Or Google Gorgon Ward Book.

Regards,
Elton

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RE: [meteorite-list] Brenham Project

2006-10-21 Thread Moni Waiblinger-Seabridge

And thank you for sharing it all with us Mr. Mani and Steve!
Wonderful achievements!

Sincerely, Moni


From: Philip mani [EMAIL PROTECTED]
To: Meteorite-list@meteoritecentral.com
Subject: [meteorite-list] Brenham Project
Date: Sat, 21 Oct 2006 09:13:47 -0500

This letter is my first post to the Meteorite List after being a long-time 
reader.  I am the fortunate beneficiary of much recognition from so many of 
you related to my Brenham Project with Steve Arnold.  Thank you for your 
kind words and encouragements.  With this posting, I wanted to publicly 
recognize certain individuals who are the main contributors, in my opinion, 
to our most recent expedition and without whose efforts and creativity the 
wonderful story written by Associated Press would not have been possible.




It was last July when I began conversations with Carolyn Sumners, Director 
of Astronomy of the Houston Museum of Natural Science.  I offered HMNS an 
opportunity to join Steve and I in Kansas on a meteorite search and 
recovery project.  Mrs. Sumners was excited about the opportunity and asked 
me what specifically HMNS could contribute as far as unanswered questions 
about the find.  I told her we questioned the timing/age-date assigned to 
the fall and we wished to try to pin-down its timing.  We discussed several 
methods for age-dating and left her and her experts to further discuss and 
implement the methods for age-dating.  A second question is the direction 
of the meteorite fall, specifically, its bearing and descent angle.  This 
question is more complex and we felt we needed to gather as much survey 
information as possible without disturbing the meteorites and the soil 
around them.  At this point, Mrs. Sumners contacted Dr. Essam Heggy with 
the Lunar Planetary Institute regarding his ground penetrating radar work.




I informed Steve and he said he would do his best for the museum.  I 
remained convinced he could find another meteorite.




After all details with the HMNS, LPI, and our landowners were worked out, I 
contacted our good friend, Darryl Pitt, to assist with all facets for 
release of information to the public regarding this expedition.




You all know our results.



Steve was able to pull the golden rabbit out of the hat.  My sincere 
appreciation and congratulations to him once again and, if you have seen 
the strewnfield you understand why.  He tells me he feels his ability to do 
so again from this point on will be less and less.  Therefore, our search 
and recovery efforts for Brenham meteorites is beginning to wind-up.




Carolyn Sumners' group from HMNS included astronomers, geologists, 
paleontologists and archeologists with long and storied excavation and 
recovery experiences.  It was a joy and a treat to be an observer of their 
efforts.  I am excited for them and their unique meteorite recovery.  Good 
going.




 Dr. Heggy, with LPI, was faced with a substantial change of conditions 
from those he originally anticipated in the field.  Southwest Kansas had 
received quite a bit of rain and in the last three days, we were in 
constant heavy drizzle, blown sideways by 20-plus mile an hour winds.  If 
not for the excitement of the project and all involved, it would have been 
miserable to be in such conditions for the 12 or more hours per day.  Dr.  
Heggy adapted his equipment and techniques and continued to proceed as 
diligently as the rest of us without becoming discouraged.  His efforts too 
were rewarded.




Finally, but certainly not least, Darryl Pitt single-handedly prepared the 
initial press release and then he, along with the brilliant efforts of a 
colleague of his in New York, facilitated the amazing Associated Press 
story by Roxana Hegeman.  Darryl worked closely with Roxana a day or two 
before Monday's final excavation of the museum's 154-pound pallasite and 
she was very well prepared for what to expect on the final day.  It was 
only yesterday evening I learned that Roxana's story has enjoyed the widest 
world-wide distribution of any story ever pertaining to meteorites (with 
the exception of the announcement of ALH84001).  Certainly amazing.




I am grateful to be a part of the Brenham Project.  I have learned much 
more than I ever anticipated being a meteorite collector.  This particular 
chapter of our project was such a treat to watch unfold.  I am reminded of 
Greg's words to the List that this is an awesome story where meteorite 
hunters, collectors and scientists can join to work together closely in the 
field using new equipment to make a wonderful meteorite recovery.  I am 
blessed to have participated.




Congratulations to Carolyn Sumners and her HMNS team for their thoughtful 
work and the additional, continuing work to come both in age-dating the 
fall and hopefully determining the fall direction and angle.




Great-going Dr. Heggy for your successful use and application of the GPR.



Hats-off to Darryl for facilitating the AP wire story or, as I